Resolving a Candidate Dual Active Galactic Nucleus with ∼100 Pc Separation in MCG-03-34-64

Anna Trindade Falcao,T. J. Turner,S. B. Kraemer,J. Reeves,V. Braito,H. R. Schmitt, L. Feuillet

The Astrophysical Journal（2024）

Harvard Smithsonian Ctr Astrophys | Eureka Sci Inc | Catholic Univ Amer | Naval Res Lab

Cited 0|Views9

Abstract

We report the serendipitous multiwavelength discovery of a candidate dual black hole system with a separation of ∼100 pc, in the gas-rich luminous infrared galaxy MCG-03-34-64 ( z = 0.016). Hubble Space Telescope/Advanced Camera for Surveys observations show three distinct optical centroids in the [O iii ] narrow-band and F814W images. Subsequent analysis of Chandra/ACIS data shows two spatially resolved peaks of equal intensity in the neutral Fe K α (6.2–6.6 keV) band, while high-resolution radio continuum observations with the Very Large Array at 8.46 GHz (3.6 cm band) show two spatially coincident radio peaks. Fast shocks as the ionizing source seem unlikely, given the energies required for the production of Fe K α . If confirmed, the separation of ∼100 pc would represent the closest dual active galactic nuclei reported to date with spatially resolved, multiwavelength observations.

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Key words

AGN host galaxies,Seyfert galaxies,High energy astrophysics

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